Antideuterons from supersymmetric dark matter

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dc.creatorDonato, F.
dc.creatorFornengo, N.
dc.creatorMaurin, D.
dc.date2007-09-13
dc.date.accessioned2026-07-07T08:29:21Z
dc.date.available2026-07-07T08:29:21Z
dc.descriptionWe calculate the antideuteron flux expected from dark matter annihilation in the galactic halo. The propagation is treated in a full 2-D propagation model consistent with the results obtained from the propagation of B/C and other galactic species. We discuss the potentials of this indirect dark matter detection means, with special emphasis on the possible sources of uncertainties affecting future measurements
dc.description4 pages, 4 figures, Proc. of the 30th International Cosmic Ray Conference, July 3 - 11, 2007, Merida, Yucatan, Mexico (ICRC07)
dc.identifierhttps://arxiv.org/abs/0709.2098
dc.identifierhttp://arxiv.org/abs/0709.2098
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/137938
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Phenomenology
dc.titleAntideuterons from supersymmetric dark matter
dc.typetext

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